Dust Devil and Gustnado
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Soaring Weather
Chapter 16 SOARING WEATHER While horse racing may be the "Sport of Kings," of the craft depends on the weather and the skill soaring may be considered the "King of Sports." of the pilot. Forward thrust comes from gliding Soaring bears the relationship to flying that sailing downward relative to the air the same as thrust bears to power boating. Soaring has made notable is developed in a power-off glide by a conven contributions to meteorology. For example, soar tional aircraft. Therefore, to gain or maintain ing pilots have probed thunderstorms and moun altitude, the soaring pilot must rely on upward tain waves with findings that have made flying motion of the air. safer for all pilots. However, soaring is primarily To a sailplane pilot, "lift" means the rate of recreational. climb he can achieve in an up-current, while "sink" A sailplane must have auxiliary power to be denotes his rate of descent in a downdraft or in come airborne such as a winch, a ground tow, or neutral air. "Zero sink" means that upward cur a tow by a powered aircraft. Once the sailcraft is rents are just strong enough to enable him to hold airborne and the tow cable released, performance altitude but not to climb. Sailplanes are highly 171 r efficient machines; a sink rate of a mere 2 feet per second. There is no point in trying to soar until second provides an airspeed of about 40 knots, and weather conditions favor vertical speeds greater a sink rate of 6 feet per second gives an airspeed than the minimum sink rate of the aircraft. -
Large-Eddy Simulations of Dust Devils and Convective Vortices
Large-Eddy Simulations of Dust Devils and Convective Vortices Aymeric Spiga, Erika Barth, Zhaolin Gu, Fabian Hoffmann, Junshi Ito, Bradley Jemmett-Smith, Martina Klose, Seiya Nishizawa, Siegfried Raasch, Scot Rafkin, et al. To cite this version: Aymeric Spiga, Erika Barth, Zhaolin Gu, Fabian Hoffmann, Junshi Ito, et al.. Large-Eddy Simulations of Dust Devils and Convective Vortices. Space Science Reviews, Springer Verlag, 2016, 203, pp.245 - 275. 10.1007/s11214-016-0284-x. hal-01457992 HAL Id: hal-01457992 https://hal.sorbonne-universite.fr/hal-01457992 Submitted on 6 Feb 2017 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Large-Eddy Simulations of dust devils and convective vortices Aymeric Spiga∗1, Erika Barth2, Zhaolin Gu3, Fabian Hoffmann4, Junshi Ito5, Bradley Jemmett-Smith6, Martina Klose7, Seiya Nishizawa8, Siegfried Raasch9, Scot Rafkin10, Tetsuya Takemi11, Daniel Tyler12, and Wei Wei13 1 Laboratoire de M´et´eorologieDynamique, UMR CNRS 8539, Institut Pierre-Simon Laplace, Sorbonne Universit´es,UPMC Univ Paris 06, Paris, France 2SouthWest -
ESSENTIALS of METEOROLOGY (7Th Ed.) GLOSSARY
ESSENTIALS OF METEOROLOGY (7th ed.) GLOSSARY Chapter 1 Aerosols Tiny suspended solid particles (dust, smoke, etc.) or liquid droplets that enter the atmosphere from either natural or human (anthropogenic) sources, such as the burning of fossil fuels. Sulfur-containing fossil fuels, such as coal, produce sulfate aerosols. Air density The ratio of the mass of a substance to the volume occupied by it. Air density is usually expressed as g/cm3 or kg/m3. Also See Density. Air pressure The pressure exerted by the mass of air above a given point, usually expressed in millibars (mb), inches of (atmospheric mercury (Hg) or in hectopascals (hPa). pressure) Atmosphere The envelope of gases that surround a planet and are held to it by the planet's gravitational attraction. The earth's atmosphere is mainly nitrogen and oxygen. Carbon dioxide (CO2) A colorless, odorless gas whose concentration is about 0.039 percent (390 ppm) in a volume of air near sea level. It is a selective absorber of infrared radiation and, consequently, it is important in the earth's atmospheric greenhouse effect. Solid CO2 is called dry ice. Climate The accumulation of daily and seasonal weather events over a long period of time. Front The transition zone between two distinct air masses. Hurricane A tropical cyclone having winds in excess of 64 knots (74 mi/hr). Ionosphere An electrified region of the upper atmosphere where fairly large concentrations of ions and free electrons exist. Lapse rate The rate at which an atmospheric variable (usually temperature) decreases with height. (See Environmental lapse rate.) Mesosphere The atmospheric layer between the stratosphere and the thermosphere. -
NCAR Annual Scientific Report Fiscal Year 1985 - Link Page Next PART0002
National Center for Atmospheric Research Annual Scientific Report Fiscal Year 1985 Submitted to National Science Foundation by University Corporation for Atmospheric Research March 1986 iii CONTENTS INTRODUCTION ............... ............................................. v ATMOSPHERIC ANALYSIS AND PREDICTION DIVISION ............... 1 Significant Accomplishments........................ 1 AAP Division Office................................................ 4 Mesoscale Research Section . ........................................ 8 Climate Section........................................ 15 Large-Scale Dynamics Section....................................... 22 Oceanography Section. .......................... 28 ATMOSPHERIC CHEMISTRY DIVISION................................. .. 37 Significant Accompl i shments........................................ 38 Precipitation Chemistry, Reactive Gases, and Aerosols Section. ..................................39 Atmospheric Gas Measurements Section............................... 46 Global Observations, Modeling, and Optical Techniques Section.............................. 52 Support Section.................................................... 57 Di rector' s Office. * . ...... .......... .. .. ** 58 HIGH ALTITUDE OBSERVATORYY .. .................. ............... 63 Significant Accomplishments .......... .............................. 63 Coronal/Interplanetary Physics Section ....................... 64 Solar Variability and Terrestrial Interactions Section........................................... 72 Solar -
The Dryline______1900 English Road, Amarillo, TX 79108 806.335.1121
TThhee DDrryylliinnee The Official Newsletter of the National Weather Service in Amarillo TEXAS COUNTY EARNS Summer STORMREADY® RECOGNITION 2008 FROM TORNADOES TO FLOODS, TEXAS COUNTY IS PREPARED By Steve Drillette, Warning Coordination Meteorologist Tornadoes, Landspouts and Texas County was presented with a NOAA National Weather Service Dust Devils – Certificate recognizing local officials and citizens for their efforts in Page 2 earning the distinguished StormReady® designation. The ceremony was held April 7, 2008 at the County Courthouse in Guymon. Texas Flood Safety – th County became the 11 StormReady Community to be recognized Page 4 across the Texas and Oklahoma Panhandles since our first community was recognized in 2002. Weather Review The ceremony was led by Jose Garcia, Meteorologist-In-Charge of the and Outlook – National Weather Service office in Amarillo. Mr. Garcia presented Page 6 Texas County Emergency Manager, Harold Tyson, with a StormReady® certificate and two StormReady® highway signs. Mr. In YOUR Kevin Starbuck, Emergency Management Coordinator of Amarillo and Community – member of the Amarillo StormReady® Advisory Board, also Page 7 participated in the presentation. Guymon Emergency Manager Clark Purdy, several county commissioners and other local officials were also on hand to accept the awards. NWS OFFICE FAREWELLS – StormReady® is a voluntary program, and is offered as a means of Page 8 providing guidance and incentive to local and county officials interested in improving hazardous weather operations. To receive StormReady® recognition, communities are required to meet minimum criteria in hazardous weather preparedness, as established through a partnership of the NWS and federal, state, and local emergency management professionals. ―Texas County officials are to be commended for their efforts in meeting and exceeding the StormReady® criteria,‖ said Mr. -
Near-Surface Vortex Structure in a Tornado and in a Sub-Tornado-Strength Convective-Storm Vortex Observed by a Mobile, W-Band Radar During VORTEX2
VOLUME 141 MONTHLY WEATHER REVIEW NOVEMBER 2013 Near-Surface Vortex Structure in a Tornado and in a Sub-Tornado-Strength Convective-Storm Vortex Observed by a Mobile, W-Band Radar during VORTEX2 ,1 # @ ROBIN L. TANAMACHI,* HOWARD B. BLUESTEIN, MING XUE,* WEN-CHAU LEE, & & @ KRZYSZTOF A. ORZEL, STEPHEN J. FRASIER, AND ROGER M. WAKIMOTO * Center for Analysis and Prediction of Storms, and School of Meteorology, University of Oklahoma, Norman, Oklahoma # School of Meteorology, University of Oklahoma, Norman, Oklahoma @ National Center for Atmospheric Research, Boulder, Colorado & Microwave Remote Sensing Laboratory, University of Massachusetts, Amherst, Amherst, Massachusetts (Manuscript received 14 November 2012, in final form 22 May 2013) ABSTRACT As part of the Second Verification of the Origins of Rotation in Tornadoes Experiment (VORTEX2) field campaign, a very high-resolution, mobile, W-band Doppler radar collected near-surface (#200 m AGL) observations in an EF-0 tornado near Tribune, Kansas, on 25 May 2010 and in sub-tornado-strength vortices near Prospect Valley, Colorado, on 26 May 2010. In the Tribune case, the tornado’s condensation funnel dissipated and then reformed after a 3-min gap. In the Prospect Valley case, no condensation funnel was observed, but evidence from the highest-resolution radars in the VORTEX2 fleet indicates multiple, sub-tornado-strength vortices near the surface, some with weak-echo holes accompanying Doppler velocity couplets. Using high-resolution Doppler radar data, the authors document the full life cycle of sub- tornado-strength vortex beneath a convective storm that previously produced tornadoes. The kinematic evolution of these vortices, from genesis to decay, is investigated via ground-based velocity track display (GBVTD) analysis of the W-band velocity data. -
Fish & Wildlife Branch Research Permit Environmental Condition
Fish & Wildlife Branch Research Permit Environmental Condition Standards Fish and Wildlife Branch Technical Report No. 2013-21 December 2013 Fish & Wildlife Branch Scientific Research Permit Environmental Condition Standards First Edition 2013 PUBLISHED BY: Fish and Wildlife Branch Ministry of Environment 3211 Albert Street Regina, Saskatchewan S4S 5W6 SUGGESTED CITATION FOR THIS MANUAL: Saskatchewan Ministry of Environment. 2013. Fish & Wildlife Branch scientific research permit environmental condition standards. Fish and Wildlife Branch Technical Report No. 2013-21. 3211 Albert Street, Regina, Saskatchewan. 60 pp. ACKNOWLEDGEMENTS: Fish & Wildlife Branch scientific research permit environmental condition standards: The Research Permit Process Renewal working group (Karyn Scalise, Sue McAdam, Ben Sawa, Jeff Keith and Ed Beveridge) compiled the information found in this document to provide necessary information regarding species protocol environmental condition parameters. COVER PHOTO CREDITS: http://www.freepik.com/free-vector/weather-icons-vector- graphic_596650.htm CONTENT PHOTO CREDITS: as referenced CONTACT: [email protected] COPYRIGHT Brand and product names mentioned in this document are trademarks or registered trademarks of their respective holders. Use of brand names does not constitute an endorsement. Except as noted, all illustrations are copyright 2013, Ministry of Environment. ii Contents Introduction ....................................................................................................................... -
DUST DEVIL METEOROLOGY Jack R
NOAA~NWS /1(}q, 3~;).. ~ . NOAA Technicai ·Memoran_dlim Nws·CR-42 U.S. DEPARTMENT OF COMMERCE National Oceanic and Atmospheric Adminlstretian National Weather Service DUST 1DEV-IL... ,. METEOROLOGY.. .. ... .... - 1!. Jack ,R. .Cooley \ i ,. CiHTRAL REGION Kansas City.. Mo. () U. S. DEPARTMENT OF COMMERCE NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION NATIONAL WEATHER SERVICE NOAA Technical Memoran:l.um NWS CR-42 Il.JST DEVIL METEOROLOGY Jack R. Cooley CENTRAL REJJION KANSAS CITY, MISSOORI May 1971 CONTENTS () l. Page No. INTRODUCTION 1 1.1 Some Early Accounts of Dust Devils 1 1.2 Definition 2 1.3 The Atmospheric Circulation Family 2 1.4 Other Similar Small-Scale Circulations 2 1.41 Small Waterspouts 3 l. 42 Whirlies 3 1.43 Fire 1-!hirhdnds 3 1.44 Whirlwinds Associated With Cold Fronts 4 l. 5 Damage Caused by Dust Devils 4 1.51 Dust DeVils Vs. Aircraft Safety 5 2. FORMATION 5 2.1 Optimum Locations (Macro and Micro) 5 2.2 Optimum Time of Occurrence (During Day and Year) 6 2.3 Conditions Favoring Dust Devil Formation 7 2.31 Factors Favoring Steep Lapse Rates Near the Ground 7 A. Large Incident Solar Radiation Angles 7 B. Minimum Cloudiness 7 C. Lmr Humidity 8 D. Dry Barren Soil 8 E. Surface Winds Below a Critical Value 9 2.32 Potential Lapse Rates Near the Ground 9 2.33 Favorable Air Flow 12 2 ,34 Abundant Surface Material 12 2.35 Level Terrain 13 2.4 Triggering Devices 13 2.5 Size and Shape 14. 2.6 Dust Size·and Distribution 14 2.7 Duration 15 2.8 Direction of Rotation 16 2.9 Lateral Speed and Direction of Movement 17 3. -
Download the Acquired Data Or to Fix Possible Problem
Università degli Studi di Napoli Federico II DOTTORATO DI RICERCA IN FISICA Ciclo 30° Coordinatore: Prof. Salvatore Capozziello Settore Scientifico Disciplinare FIS/05 Characterisation of dust events on Earth and Mars the ExoMars/DREAMS experiment and the field campaigns in the Sahara desert Dottorando Tutore Gabriele Franzese dr. Francesca Esposito Anni 2014/2018 A birbetta e giggione che sono andati troppo veloci e a patata che invece adesso va piano piano Summary Introduction ......................................................................................................................... 6 Chapter 1 Atmospheric dust on Earth and Mars............................................................ 9 1.1 Mineral Dust ....................................................................................................... 9 1.1.1 Impact on the Terrestrial land-atmosphere-ocean system .......................... 10 1.1.1.1 Direct effect ......................................................................................... 10 1.1.1.2 Semi-direct and indirect effects on the cloud physics ......................... 10 1.1.1.3 Indirect effects on the biogeochemical system .................................... 11 1.1.1.4 Estimation of the total effect ............................................................... 11 1.2 Mars .................................................................................................................. 12 1.2.1 Impact on the Martian land-atmosphere system ......................................... 13 1.3 -
Storm Spotting – Solidifying the Basics PROFESSOR PAUL SIRVATKA COLLEGE of DUPAGE METEOROLOGY Focus on Anticipating and Spotting
Storm Spotting – Solidifying the Basics PROFESSOR PAUL SIRVATKA COLLEGE OF DUPAGE METEOROLOGY HTTP://WEATHER.COD.EDU Focus on Anticipating and Spotting • What do you look for? • What will you actually see? • Can you identify what is going on with the storm? Is Gilbert married? Hmmmmm….rumor has it….. Its all about the updraft! Not that easy! • Various types of storms and storm structures. • A tornado is a “big sucky • Obscuration of important thing” and underneath the features make spotting updraft is where it forms. difficult. • So find the updraft! • The closer you are to a storm the more difficult it becomes to make these identifications. Conceptual models Reality is much harder. Basic Conceptual Model Sometimes its easy! North Central Illinois, 2-28-17 (Courtesy of Matt Piechota) Other times, not so much. Reality usually is far more complicated than our perfect pictures Rain Free Base Dusty Outflow More like reality SCUD Scattered Cumulus Under Deck Sigh...wall clouds! • Wall clouds help spotters identify where the updraft of a storm is • Wall clouds may or may not be present with tornadic storms • Wall clouds may be seen with any storm with an updraft • Wall clouds may or may not be rotating • Wall clouds may or may not result in tornadoes • Wall clouds should not be reported unless there is strong and easily observable rotation noted • When a clear slot is observed, a well written or transmitted report should say as much Characteristics of a Tornadic Wall Cloud • Surface-based inflow • Rapid vertical motion (scud-sucking) • Persistent • Persistent rotation Clear Slot • The key, however, is the development of a clear slot Prof. -
Large-Scale Extratropical Cyclogenesis and Frontal Waves: Effects on Mars Dust
Workshop on Planetary Atmospheres (2007) 9077.pdf LARGE-SCALE EXTRATROPICAL CYCLOGENESIS AND FRONTAL WAVES: EFFECTS ON MARS DUST. J.L. Hollingsworth1, M.A. Kahre1, R.M. Haberle1, 1Space Science and Astrobiology Division, Planetary Systems Branch, NASA Ames Research Center, Moffett Field, CA 94035, ([email protected]). Introduction: Mars reveals similar, yet also vastly scimitar-shaped dust fronts in the northern extratropi- different, atmospheric circulation patterns compared to cal and subtropical environment during late autumn and those found on Earth [1]. Both planets exhibit ther- early spring [8,9]. mally indirect (i.e., eddy-driven) Ferrel circulation cells Results: The time and zonally-averaged tempera- inmiddleandhighlatitudes. Duringlateautumnthrough tureandzonalwindfieldfromourbaselinehigh-resolution early spring, Mars’ extratropics indicateintense equator- (i.e., 2.0 × 3.0◦ longitude-latitude) simulation is shown to-pole temperature contrasts (i.e., mean “baroclinic- in Fig. 1. The mean zonal temperatures appear rather ity”). From data collected during the Viking era and re- symmetric about the equator. Upon closer inspection, it cent observationsfromtheMarsGlobal Surveyor(MGS) can be seen that in the northern extratropics the north- mission, such strong temperature contrasts supports in- south temperature contrasts at this season, particularly tense eastward-traveling weather systems (i.e., transient near the surface, are significantly stronger than in the synoptic-period waves) [2,3,4] associated with the dy- southern hemisphere. This asymmetry in mean zonal namical process of baroclinic instability. The travel- fields is also apparent in the mean zonal wind (Fig. 1, ing disturbances and their poleward transports of heat bottom) where the northern hemisphere’s westerly po- and momentum, profoundly influence the global atmo- lar vortex is roughly twice as strong than in the south, spheric energy budget. -
Presentation
5.4 A SUMMARY OF DATA COLLECTED DURING VORTEX2 BY MWR-05XP/TWOLF, UMASS X-POL, AND THE UMASS W-BAND RADAR Howard B. Bluestein*, M. M. French, J. B. Houser, J. C. Snyder, R. L. Tanamachi School of Meteorology, University of Oklahoma, Norman I. PopStefanija and C. Baldi ProSensing, Inc., Amherst, Massachusetts G. D. Emmitt Simpson Weather Associates, Charlottesville, Virginia V. Venkatesh, K. Orzel, and S. J. Frasier Microwave Remote Sensing Laboratory, University of Massachusetts, Amherst R. T. Bluth CIRPAS, Naval Postgraduate School, Monterey, California 1. INTRODUCTION During VORTEX2, three scanning, mobile, truck-mounted Doppler radars and a mobile, scanning Doppler lidar were used in the field by a group of faculty and graduate students from the University of Oklahoma (OU), supported by personnel from the institutions given above. These platforms were part of the VORTEX2 armada. A scout car from OU assisted with field operations. The U. Mass. W-band radar (Fig. 1) (e.g., Bluestein et al. 2007a) has been used since 1993. It has a half-power beamwidth of 0 0.18 and is used mainly to probe tornadoes Figure 1. U. Mass. W-band radar probing a at high spatial resolution, near the ground, tornado in Goshen County, Wyoming on 5 June from a range of 10 - 15 km or less. 2009. © R. Tanamachi The U. Mass. X-Pol radar (Fig. 2) is an X- band, polarimetric radar, whose antenna has identify polarimetric signatures in supercells 0 a half-power beamwidth of 1.25 . It has (Snyder et al. 2010). been used since 2001 without Doppler or The MWR-05XP (Fig.